Advanced analysis and event reconstruction for the CTA Observatory
Y. Becherini, B. Kh\'elifi, S. Pita, M. Punch (for the CTA Consortium)

TL;DR
This paper discusses advanced data analysis techniques for the CTA gamma-ray observatory, improving event reconstruction and gamma/hadron separation to enhance sensitivity over current methods.
Contribution
It introduces the Paris-MVA analysis method, combining Hillas parameters, 3D-Model algorithms, and Boosted Decision Trees for improved performance in CTA data analysis.
Findings
Sensitivity improved by a factor of about 2
Effective gamma/hadron separation achieved
Algorithms successfully applied to H.E.S.S. data
Abstract
The planned Cherenkov Telescope Array (CTA) is a future observatory for very-high-energy (VHE) gamma-ray astronomy composed of one site per hemisphere. It aims at 10 times better sensitivity, a better angular resolution and wider energy coverage than current installations such as H.E.S.S., MAGIC and VERITAS. In order to achieve this level of performance, both the design of the telescopes and the analysis algorithms are being studied and optimized within the CTA Monte-Carlo working group. Here, we present ongoing work on the data analysis for both the event reconstruction (energy, direction) and gamma/hadron separation, carried out within the HAP (H.E.S.S. Analysis Package) software framework of the H.E.S.S. collaboration, for this initial study. The event reconstruction uses both Hillas-parameter-based algorithms and an improved version of the 3D-Model algorithm. For the gamma/hadron…
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